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Curiosity Blog, Sols 4982–4987: Back to Our Regularly Scheduled Programming
NASA’s Mars rover Curiosity acquired this image, of thin, ledge-like layers at target “Los Toldos,” using its Right Mast Camera (Mastcam). Curiosity captured the image on Aug. 12, 2026 — Sol 4982, or Martian day 4,982 of the Mars Science Laboratory mission — at 01:05:04 UTC.
NASA/JPL-Caltech/MSSS
By Allison Dries-Padilla, Missions Operations Specialist at Malin Space Science Systems
Earth planning date: Friday, Aug. 14, 2026
This week of Curiosity Mars rover operations takes us back to our “regularly scheduled programming.” After taking a slight detour to investigate the “erosional surface” we are back on course to ascend Mount Sharp. As we transition into fall in Gale Crater, temperatures and the likelihood of dust storms begins to drop, but Curiosity is still on the lookout for the last gasp of late-season local and regional dust storms.
Monday’s plan for Sols 4982 to 4985 began with Curiosity standing face to face with a unique geologic feature just above the erosional supersurface contact. As you might have read in the previous blog, the team was fortunate enough to spend two planning cycles at this amazing location. MAHLI used this opportunity to reacquire selected images for the mosaic of target “Tres Morros.” This will allow the science team to have a detailed and focused view of the underside of this feature. APXS took measurements of the bedrock target “El Motacusal” after it had been brushed with the DRT. APXS took a second measurement on the “as is” bedrock target “Alto de Carmen.” Both of these APXS targets were documented with high-resolution images taken by MAHLI. ChemCam activities include LIBS spectroscopy on bedrock targets “Lagunas Bravas” and “Parququcha” and ChemCam Remote Micro-Imaging on Mishe Mokwa. I had the pleasure to be on the Mastcam uplink shift for this plan. Mastcam took a near-field mosaic of the erosional ridge, dubbed “Los Toldos,” as well as a mosaic on further away bedrock exposure above the erosional surface, named “Los Ladrillos.” In addition to these mosaics, Mastcam also provided color documentation of the previous plan’s ChemCam Remote Micro-Imaging on Cordillera and the ChemCam LIBS activities taken in this plan.
Curiosity then drove 100 feet (30 meters) to take us to our location for Friday’s plan for Sols 4985 to 4987. Although we had plenty of flat and tasty bedrock in this new location, we could not place the robotic arm in a safe position to DRT the bedrock. The left-front wheel was perched on a small rock, and we had to account for a risk the rover could slip off this rock as we move the arm around. MAHLI and APXS were still able to safely perform contact science on two bedrock targets, “Mamorecillo” and “Aguas Claras.” MAHLI had an additional housekeeping activity to image the calibration target. ChemCam plans to use its laser spectrometer to gather geochemistry on three targets in this vicinity, followed by Mastcam documentation. Today’s ChemCam LIBS targets include a dark-toned resistant layer in the bedrock “Yura Kasa.” Mastcam is planning a series of mosaics to continue imaging the stratigraphy in the unit above the erosional contact.
Today’s plan was packed with environmental monitoring activities to monitor for dust storms. Mastcam took a flurry of dust-imaging observations to measure optical depth, or “tau,” of the atmosphere. A higher tau value is associated with an increased amount of dust in the atmosphere. APXS joined in on the action by planning an overnight atmospheric measurement. Navcam took on most of the heavy lifting to monitor for dust storms. These activities include multiple large dust-****** surveys, zenith observation, in-crater line-of-sight observations, and suprahorizon cloud movies.
Curiosity will then continue to climb Mount Sharp; the planned drive distance of 150 feet (47 meters) will take the rover southwest of our current location. We will return Monday to start a new week full of contact science, remote sensing, and driving on Mars.
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NASA’s Curiosity rover at the base of Mount Sharp
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Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
Mostly Perseids
Explanation: Recorded the night of August 12-13, images from four dedicated meteor-monitoring cameras at an astronomical observatory in Czechia were aligned and combined to create this all-night, all-sky view. On that night, the total count came to 1,706 meteors. And since that coincided with the peak activity of the 2026 Perseid Meteor Shower, most are perseids. Their overwhelming numbers make them easy to spot. Quite convincingly, perseid trails all trace back to a single radiant on the sky at the upper right, a region in the annual shower’s eponymous constellation Perseus. But meteors belonging to other much less active showers can be revealed by finding their radiants too. For example, seen crossing the perseid trails are meteors from a shower whose radiant lies in Cygnus, known as Kappa Cygnids. The antihelion complex, a general region near Aquarius and opposite the Sun in the sky, is also identifiable as a weak source for meteors.
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NASA Shares Views of August Solar Eclipse from Ground, Air, Space
This composite image shows the progression of a total solar eclipse as the Sun sets over San Millán de los Caballeros, Spain, on Wednesday, Aug. 12, 2026.
Credits:
NASA/Bill Ingalls
On Aug. 12, a total solar eclipse darkened skies over Greenland, Iceland, and Spain. As the Moon covered the Sun, it briefly revealed the Sun’s wispy outer atmosphere — the corona — to those in the path of totality who were lucky enough to have clear skies. NASA researchers and photographers were along the eclipse path to study the corona, capture the phenomenon, and observe how the eclipse affected our planet.
One NASA photographer in Spain captured the total solar eclipse as well as the partial phases before and after, until the Sun set below the horizon.
This composite image shows the progression of a total solar eclipse over a field of sunflowers in San Millán de los Caballeros, Spain, on Aug. 12, 2026. Credit: NASA/Bill Ingalls
The solar corona appears in this photograph of a total solar eclipse captured from San Millán de los Caballeros, Spain, on Aug. 12, 2026. Credit: NASA/Bill Ingalls
A solar prominence, a plume of electrically charged gas suspended above the Sun by strong magnetic forces, appears as a pink feature along the left edge of the eclipsed Sun in this photograph taken from San Millán de los Caballeros, Spain, on Aug. 12, 2026. Credit: NASA/Bill Ingalls
This composite image shows the progression of a total solar eclipse as the Sun sets in San Millán de los Caballeros, Spain, on Aug. 12, 2026. Credit: NASA/Bill Ingalls
In northern Maine, where only a partial eclipse was visible, another NASA photographer captured the International Space Station, with its crew of seven aboard, speeding past the partially eclipsed Sun.
In this image of a partial solar eclipse, which is veiled by clouds, the International Space Station, with a crew of seven aboard, appears in silhouette as it transits at roughly five miles per second on Aug. 12, 2026, as seen near Hodgdon, Maine. Aboard the station as part of Expedition 75 are NASA astronauts Jessica Meir, Anil Menon, and Jack Hathaway; ESA (European Space Agency) astronaut Sophie Adenot; and Roscosmos cosmonauts Pyotr Dubrov, Andrey Fedyaev, and Anna Kikina. Credit: NASA/Joel Kowsky
Twelve frames assembled in sequence show the International Space Station, with a crew of seven aboard, in silhouette as it transits the Sun at roughly five miles per second during a partial solar eclipse on Aug. 12, 2026, as seen near Hodgdon, Maine. Clouds partially obscure the view of the Sun. Aboard the station as part of Expedition 75 are NASA astronauts Jessica Meir, Anil Menon, and Jack Hathaway; ESA (European Space Agency) astronaut Sophie Adenot; and Roscosmos cosmonauts Pyotr Dubrov, Andrey Fedyaev, and Anna Kikina. Credit: NASA/Joel Kowsky
Meanwhile, from about 250 miles above the ground, a NASA astronaut aboard the International Space Station snapped a few photos of the partial eclipse from their perspective as well.
NASA astronaut Jessica Meir captured this photo of the partial solar eclipse from the International Space Station on Aug. 12, 2026, as the orbital outpost soared 262 miles above southern Quebec, Canada. From the station, the Moon covered about 18% of the Sun at the peak of the eclipse. Credit: NASA/Jessica Meir
Between the ground and the space station, NASA pilots flew NASA’s WB-57F research jet at an altitude of 50,000 feet, passing through the eclipse’s shadow to lengthen their time in the eclipse. The jet carried a suite of cameras that captured high-resolution images of the corona and prominences, plumes of electrically charged gas rising off the Sun, in several different wavelengths of light.
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The total solar eclipse on Aug. 12, 2026, was captured by a camera mounted inside the cockpit window of NASA’s WB-57F aircraft as it flew around 50,000 feet altitude off the coast of Iceland.
NASA
A suite of cameras installed on NASA’s WB-57F aircraft captured images of the solar corona and prominences in different wavelengths of visible and infrared light during the total solar eclipse on Aug. 12, 2026. A science team led by the Southwest Research Institute in Boulder, Colorado, will analyze the images to learn more about complex and dynamic features in the Sun’s outer atmosphere. Credit: NASA/SwRI/Will Ashfield
In both Iceland and Spain, teams of students participating in the NASA-funded Nationwide Eclipse Ballooning Project launched scientific balloons that carried instruments to capture images of the eclipse’s shadow and study the eclipse’s effects on our atmosphere. Even though clouds obscured the view of the eclipse from the ground in Iceland, the weather did not interfere with the balloon-borne instruments’ ability to gather information about how the brief loss of light and heat affected the lower atmosphere.
Students participating in the NASA-funded Nationwide Eclipse Ballooning Project prepare to launch a scientific balloon in Mosfellsbær, Iceland, during the total solar eclipse on Aug. 12, 2026. Credit: NASA/Abbey Interrante
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The Moon’s shadow passes over the atmosphere during the total solar eclipse on Aug. 12, 2026. The video was taken by a camera carried by a scientific balloon launched from Spain by a student team from Montana State University participating in the NASA-funded Nationwide Eclipse Ballooning Project. The video captures about six minutes of time but is sped up to play at four times real speed. Passing through the foreground are some other science instruments carried by the same balloon.
Nationwide Eclipse Ballooning Project/Montana State University
Before the eclipse, scientists at Predictive Science Inc., with support from NASA grants and supercomputers, used observations of the Sun from NASA spacecraft and ground-based telescopes to predict what the corona would look like during the eclipse. Below, their corona prediction is compared to a composite image of the corona, which combines multiple images captured by the NASA-supported DEB Initiative project during the total eclipse near León, Spain.
prediction
image
This image shows a prediction from the morning of Aug. 12, 2026, of what the solar corona would look like to the human eye during the total solar eclipse that day.
Predictive Science Inc.
This processed, composite image of the corona combines multiple images captured near León, Spain, during the total solar eclipse on Aug. 12, 2026.
DEB Initiative Team/Zack Stockbridge
predictionimage
This image shows a prediction from the morning of Aug. 12, 2026, of what the solar corona would look like to the human eye during the total solar eclipse that day.
Predictive Science Inc.
This processed, composite image of the corona combines multiple images captured near León, Spain, during the total solar eclipse on Aug. 12, 2026.
DEB Initiative Team/Zack Stockbridge
prediction
image
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Image Details
The left image shows a prediction from the morning of Aug. 12, 2026, of what the solar corona would look like to the human eye during the total solar eclipse that day. The right image is processed, composite image of the corona that combines multiple images captured near León, Spain, during the total solar eclipse on Aug. 12, 2026. Left image credit: Predictive Science Inc.; right image credit: DEB Initiative Team/Zack Stockbridge
Over the coming months, scientists will analyze the observations and images captured during the solar eclipse on Aug. 12 and present what they have learned about the Sun and its effects on our home planet. These observations will also help prepare science teams to investigate future solar eclipses, such as a much longer total solar eclipse that will be visible from southern Spain and northern Africa on Aug. 2, 2027.
Read more about NASA’s research during the eclipse and rewatch NASA’s eclipse broadcast to hear from some of the scientists and students who conducted the experiments.
About the Author
Vanessa Thomas
Vanessa Thomas is a science writer with the heliophysics communications team at NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
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NASA’s Chemical Equilibrium with Applications (CEA) code is a foundational tool for propulsion system analysis. It provides equilibrium chemistry, rocket performance, shock, and detonation calculations used across NASA and the broader aerospace community. NASA Engineering and Safety Center (NESC) Activity TI-22-01730 modernized the legacy CEA2 Fortran code into CEA v3, a Fortran 2008, object-oriented software package with expanded interface support, updated thermochemical data, improved maintainability, and substantially improved workflow integration. The modernized code preserves backward compatibility with legacy CEA input workflows while enabling direct use from modern analysis environments, including Python, C, MATLAB, and automated design studies.
Background
CEA2 was released in 2002 and has remained widely used for propulsion and thermochemistry analysis. However, the original procedural Fortran implementation became increasingly difficult to maintain, extend, and integrate into modern engineering workflows due to the lack of a subroutine interface. Current propulsion analysis increasingly requires automated parametric sweeps, integration with other modeling tools and engineering workflows, and support for emerging propellants and fuels, including green propellants and sustainable aviation fuels. These needs motivated a comprehensive modernization effort to preserve CEA’s validated technical basis while improving its maintainability, usability, and integration with modern engineering software.
Technical Improvements
Modern Software Architecture
CEA v3 is implemented in Fortran 2008 using object-oriented data structures, stricter typing, and a thread-safe equilibrium solver architecture. The software supports Fortran, C, Python, MATLAB, and Excel interfaces. These interfaces allow CEA to be used directly in automated analysis pipelines, multidisciplinary design frameworks, and high-volume designof- experiments studies. Backward compatibility is supported through a legacy command-line interface, allowing existing CEA input files and workflows to be carried forward with minimal disruption.
Expanded Species and Thermodynamic Data
The thermodynamic database has been expanded to support additional propellants and fuels relevant to current NASA applications, including green propellant constituents such as ADN, HAN, and LMP-103S, and sustainable aviation fuel candidates such as n-Butanol. This expanded species coverage improves the applicability of CEA for next-generation propulsion, green propellant, and sustainable aviation fuel studies.
New Modeling Capabilities
CEA v3 adds or improves support for several modeling capabilities, including:
Subroutine interface enabling direct integration and high-volume calculations
Negative reactant amounts
Inert hydrocarbon fuel representations, including RP-1, Jet-A, and JP-series fuels
Analytic total derivatives for coupling with optimization and sensitivity analysis workflows
Performance Improvements
For standalone use, individual equilibrium calculations in CEA v3 are moderately slower than comparable CEA2 calculations because the modernized architecture and added robustness introduce additional computational overhead. In representative testing, a single calculation was approximately 40 percent slower, but the absolute difference was only about 0.004 seconds per case. However, the modernized architecture provides substantial performance advantages for multi-case workflows, which are common in design-of-experiments studies, parametric sweeps, optimization, and uncertainty analyses. In one benchmark, a sweep of 108,500 cases completed in approximately 1.11 seconds with CEA v3, compared with approximately 15 minutes using CEA2. This corresponds to an approximately 800-times reduction in runtime for that workflow. These improvements make large-scale propulsion trade studies and automated design-space exploration significantly more practical.
Guidance for Engineering Use
NASA engineering users should consider the following guidance:
Use CEA v3 for new propulsion and thermochemistry analyses when possible to take advantage of the modernized interfaces, expanded database, and improved workflow integration.
Use the Python, MATLAB, or C interfaces for automated workflows, including parametric sweeps, optimization studies, and iterative design analyses.
Use the updated species database for green propellant and sustainable aviation fuel studies when the relevant species are included and validated for the intended application.
Use the classic command-line interface when continuity with legacy CEA workflows or input files is required.
Retain appropriate engineering review and validation when transitioning established CEA2 workflows to CEA v3, particularly for mission-critical analyses or cases that depend on legacy assumptions.
References
NASA/TM–20260007987
CEA documentation: [Hidden Content]
CEA repository: [Hidden Content]
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Image credit: ESA/Webb, NASA & CSA, M. Reiter; Acknowledgement: M. H. Özsaraç
NASA’s James Webb Space Telescope captured this Aug. 6, 2026, infrared image of part of the Carina Nebula, a star-forming region also home to the Cosmic Cliffs. This feature, called the “Treasure Chest,” is an object known as a cometary globule. A cometary globule is an isolated cloud of gas and dust with a dense, dark head and a sweeping tail.
Image credit: ESA/Webb, NASA & CSA, M. Reiter; Acknowledgement: M. H. Özsaraç
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From left, Artemis II crew NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (********* Space Agency) astronaut Jeremy Hansen are photographed on April 29, 2026, in the White House Oval Office with President Donald J. Trump.Credit: White House
President Donald J. Trump will award each of NASA’s Artemis II crew members the Congressional Space Medal of Honor at 11 a.m. EDT on Friday, Aug. 28, during a ceremony at the agency’s Johnson Space Center in Houston.
NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and CSA (********* Space Agency) astronaut Jeremy Hansen, completed a 10-day mission around the Moon on April 10. During a historic test flight as the first astronauts to fly aboard NASA’s Orion spacecraft, these crew members were the first to travel beyond the Moon in more than 50 years and traveled farther in space than humans have ever before.
NASA Administrator Jared Isaacman will join the President and astronauts in the awards ceremony.
The event will stream live on a variety of platforms. Learn how to watch online:
[Hidden Content]
In addition to pooled media, limited media credentialing is available for this event. To apply, please submit your request online by 5 p.m. CDT on Tuesday, Aug. 25.
Learn more about NASA’s Artemis program on the agency’s website.
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Bethany Stevens / Cheryl Warner Headquarters, Washington 202-358-1600 *****@*****.tld / *****@*****.tld
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LocationNASA Headquarters
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Output from NASA’s GEOS (Goddard Earth Observing System) global model shows daily maximum surface air temperature across Western Europe from May 1 to August 19, 2026. The darkest red areas indicate temperatures that met or exceeded 40°C (104°F).
NASA Earth Observatory/Lauren Dauphin
Western Europe got its first hint of an unusual summer in May 2026, when a heat dome produced exceptional temperatures that shattered records in several countries. Remarkable as it was, that early heat wave turned out to be only the opening salvo.
By mid-August, Europeans were sweating through their fifth heat wave of the season, with the latest onslaught pushing temperatures well above 40 degrees Celsius (104 degrees Fahrenheit) across a broad area. During these bouts of extreme weather, high temperatures were often unrelenting, persisting for several days and sometimes weeks on end, and remaining overnight.
For a region accustomed to relatively mild summers, the heat upended everyday life. Hospitalizations and heat-related deaths spiked. Highways and train tracks buckled, forcing road closures and service disruptions. Large and destructive wildfires raged in areas where they were once rarely seen. The heat also worsened the severe drought that has gripped the region for months, contributing to record-low river water levels and disrupting water and power supplies, transportation routes, and agriculture.
The animation above shows the daily maximum surface air temperature across Western Europe from May 1 to August 19, 2026. It was produced by combining satellite observations with temperatures predicted by a version of NASA’s GEOS (Goddard Earth Observing System) global model, which uses mathematical equations to represent physical processes in the atmosphere. The darkest red areas indicate where temperatures met or exceeded 40°C.
The heat broke records at a furious pace, often by wide margins. According to the *** Met Office, temperatures soared as high as 35.1°C (95.2°F) in London on May 26, smashing the previous May record by 2.3°C (4.1°F). In June, Bordeaux, France, broke its maximum-temperature record on three consecutive days, hitting 42.5°C on June 24, Météo-France reported. Slovakia, meanwhile, set new national records for both daytime and nighttime highs in August. Combined June and July temperatures in Western Europe were the highest on record, according to Europe’s Copernicus climate monitoring service.
In Europe, extreme temperatures collided with several vulnerabilities, including limited access to air conditioning, high nighttime temperatures, and a lack of green space in some cities. The circumstances triggered not just discomfort but heat exhaustion and heatstroke in some cases. Preliminary reports suggest that heat may have been associated with 10,000 excess deaths, including thousands of people in the ***, France, Germany, and Belgium.
“Air conditioning is an especially critical issue in Europe in the short term,” said Anamika Shreevastava, a researcher at New York University who studied urban heat islands as a postdoc at NASA’s Jet Propulsion Laboratory. One of her goals was to produce thermal maps based on NASA data from missions like ECOSTRESS that city planners could use to make cities more resilient to heat waves.
International Energy Agency data show that 23 percent of homes in Europe have air conditioning, compared to 90 percent of homes in the United States. That difference contributes to the much higher death rates that researchers have documented in European cities during heat waves than in comparable American cities. “Longer term, cities can also plant trees, expand parks, use reflective roof paint, and transition to building materials less likely to retain heat,” Shreevastava said.
An analysis from the World Health Organization indicates that heat stress is the world’s leading cause of weather-related deaths, noting it exacerbates underlying illnesses, including cardiovascular disease, diabetes, mental health conditions, and asthma. Researchers have calculated that roughly 489,000 heat-related deaths occur each year, with 45 percent of the deaths in Asia and 36 percent in Europe.
“For older adults with physical health problems, temperatures as low as 26.7°C (80°F) can pose significant danger,” said Deborah Carr, a Boston University sociologist who specializes in the study of aging. “Nighttime heat is especially harmful for older adults whose homes lack air conditioning.”
Carr is part of a research team that used demographic data, along with temperature and climate data archived by NASA, to identify which parts of the world are at the greatest risk of current and future heat exposure. Southern Europe was among the areas facing growing heat exposure and an aging population, the researchers found.
Other research, published in Lancet Planetary Health in August 2026, underscores the importance of demographics in assessing the risks posed by heat. This study, led by Stanford researcher Qinqin Kong, mapped where increasing heat is likely to lead to intolerable conditions in the coming decades for young, middle-aged, and older adults, concluding that safe thresholds will be breached often and widely, with risks falling disproportionately on older people.
“The human body can tolerate only a limited range of ambient heat,” said Kong, a recipient of a NASA Earth and Space Science and Technology award. “Understanding where, when, and to what extent these limits are exceeded is critical.”
With intolerable levels of heat expected to affect more people across larger regions and for longer periods than previously thought, Kong and his colleagues hope that their findings will inform targeted heat action plans, emergency preparedness, and health system planning.
NASA Earth Observatory image by Lauren Dauphin, using GEOS-FP data from the Global Modeling and Assimilation Office at NASA GSFC. Story by Adam Voiland.
References & Resources
AP (2026, August 10) *** and France prepare for another heat wave as western Europe sets new temperature record. Accessed August 20, 2026.
Copernicus Climate Change Service (2026, August 12) Exceptionally hot and dry conditions fuel wildfires in Europe as ocean surface temperatures reach record highs for July. Accessed August 20, 2026.
Copernicus Climate Change Service (2026, July 9) Record heatwave brings hottest June for western Europe during second-warmest June globally. Accessed August 20, 2026.
Falchetta, G., et al. (2024) Global projections of heat exposure of older adults. Nature Communications, 15, 3678.
Kong, Q., et al. (2026) Exceeding human heat tolerance in a warming, ageing world: a global projection modelling study. The Lancet Planetary Health, In press.
Met Office (2026, June 17) May 2026 temperature records verified. Accessed August 20, 2026.
NASA (2025) Global Temperature – Earth Indicator. Accessed August 20, 2026.
NASA Earthdata (2022) Training: Satellite Remote Sensing for Measuring Urban Heat Islands and Constructing Heat Vulnerability Indices. Accessed August 20, 2026.
NASA Earthdata, Heat. Accessed August 20, 2026.
The New York Times (2026, August 14) Europe Is Once Again in the Grip of a Heat Wave. Accessed August 20, 2026.
Reuters (2026) Tracking Western Europe’s heatwave. Accessed August 20, 2026.
World Meteorological Organization (2026, August 12) Record-breaking heat and extreme weather continue. Accessed August 20, 2026.
World Resources Institute (2026, June 30) Europe’s Soaring Heat and the Great Air Conditioning Dilemma. Accessed August 20, 2026.
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Join NASA in the Exhibit Hall (Booth # 635, 835, 641, and 940) for Storytelling by NASA experts. Full Agenda below.
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BryceTech’s Smallsats by the Numbers: 2026
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From Rideshare to Dedicated Launches: SmallSat Options with NASA LSP
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You Bring the Mission, We’ll Bring the Lab: Partnering with MSFC
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NASA Ames Mission Design Center: Imagining the Next Generation of Spaceflight Missions
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A jacket decorated with Artemis I and II mission patches, along with other NASA patches hangs on the back of a chair on Thursday, Aug. 6, 2026, inside the Rocco A. Petrone Launch Control Center at NASA’s Kennedy Space Center in Florida during a terminal countdown simulation for the Artemis III mission.
NASA’s Exploration Ground Systems team conducted the terminal count simulation, which runs through the final five hours of launch countdown, including terminal count – the remaining 10 minutes of the countdown. Artemis III will carry out a series of objectives in low Earth orbit designed to demonstrate critical systems needed for future lunar landings, beginning with Artemis IV.
Stay up to date with NASA’s Artemis program.
Image credit: NASA/Clayton Rougelot
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4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA has selected four university teams to help the agency transform the future of aviation through projects ranging from high-supersonic propulsion systems to low-noise routes for small aircraft flying through cities.
The agency made awards through its University Leadership Initiative, which offers student teams the opportunity to contribute to real-world flight research that advances NASA’s goals in aeronautics.
This year’s awardees are pursuing projects that align with NASA strategic objectives, including innovation in commercial high-speed aircraft, the development of new tools that can lead to transformational aviation breakthroughs, safer and more efficient air traffic management, and the integration of new air transportation options into the national airspace.
“With these four new awards, the University Innovation project is leaning in on NASA’s aeronautics mission priorities,” said Andrew Provenza, project manager, NASA’s Glenn Research Center in Cleveland. “These teams will research new propulsion concepts for supersonic flight, novel engineering methods that can revolutionize aerospace system design and certification, and learning-enabled avionics for new advanced and urban air mobility flight vehicle platforms, which could enhance air traffic control modernization.”
The awards represent the ninth round of NASA University Leadership Initiative funding.
Totaling about $30 million, NASA’s awards will provide multiyear support for awardee universities to build their teams and conduct research. The initiative provides hands-on experiences for students, developing the U.S. aeronautics research workforce while also producing findings that will help drive aviation forward.
University Leadership Initiative awards go to teams comprised of graduate and undergraduate students and led by faculty members. Recipients form academic partnerships with other universities and community colleges, as well as industry. Experts from NASA, the Federal Aviation Administration, and other organizations provide support and guidance.
The awardees are:
University of Minnesota
Adaptive Supersonic Combined Cycle Engine for Next-generation Transportation
Led by Terrence Meyer, the project will work over four years to develop a fuel-flexible propulsion system that uses a traditional jet turbofan during takeoff and subsonic flight, but would transition to a new type of ramjet engine for supersonic flight. In ramjet mode, the system would cruise at Mach 4, or more than 3,000 mph. The project aims to enable efficient, faster-than-sound flight, including flight at high-supersonic speeds.
Stanford University
Safety Across Lifecycle of Learning-Enabled Avionics Systems: Safety Data Flywheel
Led by Somil Bansal, this four-year project aims to develop an avionics system to control an aircraft’s communications, navigation, and other electronics that incorporates machine learning. The system would take an approach that ensures safety is continuously reinforced throughout its operations. This research could help create a framework for the aviation sector to safely integrate artificial intelligence-enabled avionics into the national airspace.
Stanford University
Noise-Optimal Trajectory Planning for Urban Air Mobility Operations, Including Ambient Noise
Led by Juan Alonso, the center created through this award will work over four years to develop a high-fidelity simulation framework focused on developing low-noise flight paths in urban environments for future small aircraft. Developers are envisioning urban air mobility aircraft as ways to move people and cargo over populated areas. This center would integrate realistic models of how sound travels in cities to enable vehicle flight paths that would reduce community noise exposure from new air traffic.
Virginia Tech
Certification Driven Aircraft Design Under Uncertainty
Led by Darshan Sarojini, this three-year project proposes to transform next-generation aircraft design while integrating powerful new computer modeling tools: model-based systems engineering, multidisciplinary design, analysis and optimization, and high-dimensional uncertainty quantification. The goal is safe, faster, and more efficient modeling that results in fewer costly redesigns later in the aircraft development cycle.
For more than 10 years, NASA’s University Leadership Initiative has fostered bold ideas, collaborative research, and team-led solutions. The initiative is part of NASA’s Research and Technology Mission Directorate.
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EditorLillian GipsonContactLynne Sahay*****@*****.tld
Related TermsAeronauticsAeronautics Research Mission DirectorateFlight InnovationResearch and Technology Mission DirectorateTransformative Aeronautics Concepts ProgramUniversity InnovationUniversity Leadership InitiativeUniversity Student Research Challenge
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The View from Above: The Gemini Visual Acuity Experiments
Astronauts L. Gordon Cooper Jr. and Charles “Pete” Conrad Jr. (shown here) participated in visual experiments during the Gemini V mission in August 1965.
Credits:
NASA/L. Gordon Cooper Jr.
NASA astronaut L. Gordon Cooper, Jr. took 29 color photographs of the Earth with a 70mm camera as he orbited our planet during the Mercury-Atlas 9 mission in May 1963. Cooper’s view from the window of his Faith 7 spacecraft was spectacular, and he reported that he could see vehicles motoring on dirt roads, smoke-belching trains, and the tops of houses.
Researchers and members of the public had their doubts. Could Cooper actually see objects on the Earth’s surface in such fine detail while orbiting 100 miles above the planet? Some vision experts assumed that astronauts with 20/20 vision could not clearly see objects with sides less than 150 feet long at orbital altitudes. Although Cooper reportedly had exceptional 20/12 vision, certainly he could not see a white automobile kicking up a dust cloud near the U.S.-Mexico border as he claimed. Cooper, however, was not alone in his assertions. Other Mercury astronauts also reported seeing objects on the Earth in striking detail.
During his 22-orbit Mercury-Atlas 9 spaceflight in May 1963, L. Gordon Cooper Jr. took photos from the Faith 7 spacecraft including this one showing lakes in Western Tibet.NASA
These claims caused mental health professionals to question the sanity of NASA’s first astronauts. A story in Air Force and Space Digest noted that some psychiatrists speculated that “weightlessness was causing the astronauts to hallucinate and that the space program was in for serious trouble.” While mental health experts considered the effects of space flight on the brain, visual acuity experts mulled over the Mercury astronauts’ assertions and developed an experiment to determine what they could see on Earth from space.
Putting Astronaut Vision to the Test
NASA and its partners developed two visual acuity experiments and conducted them during the crewed Gemini V and Gemini VII missions. The first experiment involved looking through an optical device reminiscent of binoculars. Test subjects looked through the eyepieces to see an assortment of rectangles in various positions and levels of contrast. They were then asked to identify the directional orientation of the rectangles.
Another part of the experiment involved creating two enormous terrestrial eye charts composed of gigantic white rectangles. The rectangles, created by the Dow Chemical Corporation, ranged in size from roughly 150 to 600 feet long. The experiment team placed one set of rectangles on dark tilled soil in Laredo, Texas and another near Carnarvon, Australia, and asked Gemini V and VII astronauts to identify their directional orientation from orbit. This visual acuity tool was nicknamed the “Eye-Q” chart.
In-Flight Vision Testing InstrumentDrawing illustrating a Gemini astronaut using the In-Flight Vision Tester.NASA
Gemini V Visual Acuity ExperimentThis illustration shows the intended orientation of the Gemini spacecraft as it orbited over the “Eye-Q” ground observation sites.NASA
Cloudy conditions, sunlight scattered by the window of the Gemini spacecraft, and unfavorable orbital orientations during overflight all impacted the astronauts’ views of the ground-based experiments. Nevertheless, during some orbital revolutions, astronauts on both missions were able to see portions of the ground site near Laredo.
Aerial view of the visual acuity experiment’s ground site in Laredo, Texas.NASA
Their reports on the Laredo “Eye-Q” site, combined with the results of the binocular-like vision tester experiments conducted before, during, and after the flight, revealed that astronauts could in fact see roads and ships with following wakes from orbit. The experiments also determined that an astronaut’s vision did not deteriorate during a two-week spaceflight.1
Astronaut Frank Borman, Gemini VII command pilot, participates in a vision experiment using the in-flight visual acuity device during the two-week mission in December 1965.NASA
Implications
Determining what features on Earth astronauts could accurately see from orbit was about much more than sanity checking astronaut reports. Understanding what human eyes could see from space, as well as seeing the photographs taken on NASA’s early crewed missions had huge implications for geologists, geographers, oceanographers, and others studying our planet.
The scientific community’s interest in the recollections and photographs of the Earth’s surface as seen by the Mercury and Gemini astronauts motivated NASA and its partners to advocate for new Earth-observing instruments. NASA, the U.S. Geological Survey, the Office of Naval Research, and the U.S. Department of Agriculture noted that surface images of the Earth captured from above could be used to inventory crops, map geological features, monitor natural disasters, and better understand the ocean’s processes.
This photograph of the San Francisco Bay area of California was taken as part of the Skylab Earth Resources Experiment Package in January 1974.NASA
The promise of these real-world applications motivated the creation of the Earth Resources Technology Satellite (ERTS), later renamed Landsat 1. Launched by NASA in 1972, the data from Landsat 1’s camera and multi-spectral scanner were used along with data from the agency’s Earth Resources Aircraft Program to monitor the oceans, agricultural fields, natural disaster sites, and more.
In the six decades since America’s first pioneering human spaceflights, NASA has continued to observe the Earth from orbit, aircraft, and even ground level in a continuing quest to help solve problems here on Earth.
Note
[1] In subsequent years, scientists have documented that roughly 70% of astronauts experience Spaceflight Associated Neuro-ocular Syndrome (SANS) during longer spaceflights.
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This map, derived from NASA’s GEOS (Goddard Earth Observing System), shows an atmospheric river reaching Washington state in December 2025, during a winter marked by extreme rainfall and too little mountain snow.NASA’s Scientific Visualization Studio
As the effects of the 2026 snow drought in the western United States carry into summer, NASA Earth data is feeding machine-learning forecasts that inform decisions about water, power, and public safety in Washington state.
Tacoma Power, a Washington public utility, is using a U.S. technology company’s river-flow forecasts during a year of water extremes on the Cowlitz River. The utility’s largest hydroelectric project uses water stored behind Mayfield and Mossyrock dams to generate enough electricity to serve more than 151,000 homes each year.
Upstream Tech’s HydroForecast combines weather forecasts and river measurements with NASA-produced satellite data on snow cover and vegetation conditions to predict river flow from hours to days ahead. Updated every two hours, the forecasts are used by reservoir managers, hydropower producers, water utilities, and government agencies to prepare for storms, plan reservoir water releases, and navigate dry periods.
“Part of NASA’s mission is to make the view from space useful on the ground,” said Erin Urquhart, manager for NASA’s Water Resources program at the agency’s headquarters in Washington, D.C. “When an American company incorporates NASA’s freely available data into forecasts that help water managers prepare for floods, generate power, and steward water supplies, that’s NASA delivering practical value to the nation.”
Year of water extremes
During the winter of 2025-26, unusual warmth meant a larger share of precipitation fell as rain instead of snow across much of the West, while below-normal precipitation deepened deficits in some areas. January, February, and March each had the lowest Western snow cover for that month in the NASA MODIS (Moderate Resolution Imaging Spectroradiometer) satellite record since 2001.
On the Cowlitz, those conditions produced a season of extremes. In December 2025, a powerful atmospheric river brought a long, narrow band of Pacific moisture into the region, causing one of the largest one-day inflow surges ever recorded at Tacoma Power’s hydroelectric project. Across the season, that rain-heavy pattern sent water downstream quickly instead of building mountain snowpack that would melt and release water steadily into summer. Snowpack remained at just 20% to 50% of normal levels.
As winter became spring, the rain tapered off, and on April 8, Washington state placed every watershed, including the Cowlitz, under a drought emergency. From April through June, peak daily inflow into the project was among the lowest on record, leaving Tacoma Power with less incoming water to replenish its reservoirs ahead of summer demand, said Saul Villarreal, Tacoma Power’s senior hydro operations manager.
Tacoma Power’s Mayfield Dam and powerhouse sit on the Cowlitz River in southwest Washington, where forecasts using NASA data support reservoir operations and hydropower generation.Tacoma Power, used with permission
Turning satellite data into river forecasts
NASA turns observations collected by the VIIRS (Visible Infrared Imaging Radiometer Suite) instrument on the Suomi-NPP (Suomi National Polar-orbiting Partnership) satellite into data products that provide information about snow cover and vegetation greenness across entire watersheds, including where ground monitors are sparse.
To train HydroForecast, Upstream Tech collects and archives years of those NASA products alongside weather forecast data and actual river-flow measurements. Using records from hundreds of watersheds, the models learn common patterns in how water moves through the landscape and apply them in new locations.
Tests across multiple basins found that including snow and vegetation observations increased forecast skill, said Dr. Laura Read, director of technical and federal partnerships for HydroForecast at Upstream Tech. “NASA’s data gives us the reliability, global coverage, and consistency we need,” said Read. “Our short-term models run every two hours, so those inputs have to show up when we need them. Though we have stopgaps in place, any interruption to our operational pipeline is a huge deal.”
Tacoma Power uses HydroForecast alongside stream gauges, snow stations, and operator judgment. During the December storm, the NASA-informed, short-term forecast helped the utility anticipate how much water would reach the project and prepare for dynamic river conditions, while meeting operating requirements and keeping public safety at the forefront, Villarreal said.
To view this video please enable JavaScript, and consider upgrading to a web browser that
supports HTML5 video NASA’s GEOS (Goddard Earth Observing System) maps an atmospheric river, a ribbon of water vapor, before Washington’s January-April 2026 snow cover is compared with a historical median.NASA’s Scientific Visualization Studio
As spring approached, the operational challenge reversed. Tacoma Power used HydroForecast’s seasonal model to track the growing risk of weak runoff and began keeping its reservoirs higher than usual to preserve water for summer. That left less space to contain another large storm, so operators continued checking the short-term forecast “to play defense,” and remained ready to adjust operations if another atmospheric river developed.
“The earlier we understand how conditions might change, the more effective planning we can do to manage our reservoir and balance the many demands of our system throughout the season,” said Villarreal.
Tacoma Power entered summer 2026 with reservoir levels near average despite the dry spring. The stored water supports reliable hydropower, required river flows to support fish and aquatic habitat, and public recreation. It also gives the utility more flexibility to meet electricity demand during heat waves or unexpected outages and, when possible, support the wider regional power system.
From forecasts to drought assessments
Tacoma Public Utilities’ Cowlitz Hydro Project is just one example of NASA science supporting water decisions across the West.
NASA also has partnered with the U.S. Department of Agriculture’s Natural Resources Conservation Service to bring satellite-based snow and groundwater information into machine-learning water-supply forecasts.
The National Oceanic and Atmospheric Administration’s Colorado Basin River Forecast Center uses MODIS and VIIRS data to adjust snowmelt rates in its model. The Bureau of Reclamation uses NASA and NASA-derived snow data, alongside other sources, for reservoir operations in California’s San Joaquin Basin.
NASA data and research have long informed the U.S. Drought Monitor, the weekly assessment used by farmers, water managers, and public agencies. NASA became a formal partner in 2026, expanding its role from providing information to helping produce the assessment. The agency took its first turn authoring the Drought Monitor during the week of Aug. 17.
Discover more about NASA’s drought work
About the AuthorEmily DeMarcoWriter/Editor (IV), Earth Science DivisionEmily is a science writer and editor with NASA’s Earth Science Division, with more than 10 years of experience in science journalism and communication. A former deputy news editor at the magazine Science News, she holds a master’s in environmental science and management from UC Santa Barbara’s Bren School, where she specialized in water resources management and science communication.
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Related TermsGoddard Space Flight CenterDroughtsEarthEarth’s AtmosphereWater on Earth
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Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
The Elephant’s Trunk in Cepheus
Explanation: Like an illustration in a galactic Just So Story, the Elephant’s Trunk Nebula winds through the emission region and young star cluster complex IC 1396, in the high and far off constellation of Cepheus. Also known as vdB 142, this cosmic elephant’s trunk is over 20 light-years long. The detailed telescopic view features the bright swept-back ridges and pockets of cool interstellar dust and gas that abound in the region. But the dark, tendril-shaped clouds contain the raw material for star formation and hide protostars within. Nearly 3,000 light-years distant, the relatively faint IC 1396 complex covers a large region on the sky, spanning over 5 degrees. Top to bottom this proboscidean-like rendition reaches across an almost 1 degree wide field of view, though. That’s a little less than the angular size of 2 full moons.
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An iceberg drifts through the Denmark Strait in this image acquired on June 12, 2026, by the OLI (Operational Land Imager) on Landsat 9.NASA Earth Observatory/Lauren Dauphin
Greenland’s jagged coastline is lined with fjords, many of them cradling marine-terminating glaciers that routinely calve icebergs into the water. It’s common to see these bergs, small and large, drifting in the island’s fjords each summer once the sea ice breaks up. In summer 2026, one exceptionally large berg turned up in the Denmark Strait—more than a thousand kilometers south of where it apparently originated.
These images, captured by the OLI (Operational Land Imager) on Landsat 9, show the iceberg on June 12 as it drifted in the strait between Greenland and Iceland. It was just south of Kangikajiip Appalia, a cape on Greenland’s east coast visible in the scene’s upper left, amid a mixture of sea ice and berg fragments known as “mélange.”
Alexis Denton, oceanographer and chief scientist with the International Ice Patrol, noted that several clues indicate it is an iceberg rather than thick, multi-year sea ice: its proximity to shore, its whiter color, and larger size compared to the surrounding sea ice. Measuring roughly 17 square kilometers (7 square miles) on June 12, the iceberg was about five times the area of New York City’s Central Park. That’s modest compared to the behemoth bergs that calve from Antarctic glaciers and ice shelves but large by Greenland standards.
Keld Quistgaard, a senior ice advisor with the Danish Meteorological Institute’s Greenland Ice Service, noted that it originated in Jøkelbugten—a bay in northeastern Greenland. The berg’s precise origin within that bay, however, remains something of a mystery. It’s possible that the berg broke off from Zachariæ Isstrøm or its adjacent remnant ice shelf. The ice shelf, which together with Zachariæ Isstrøm once filled the bay, was abandoned after the glacier rapidly retreated in the early 2000s.
Tracing its path back through satellite imagery is challenging. Through spring, the bay and surrounding coastal areas are choked with sea ice and berg fragments, making individual bergs hard to distinguish, especially if covered in bright snow. In late May, for instance, the berg was surrounded by numerous look-alikes. Only later in the season, as it drifted farther south and the ice around it thinned out, did it become distinct enough to easily spot.
The iceberg’s bright white surface is pocked with light blue meltwater ponds in this detailed view of the image, acquired on June 12, 2026, by the OLI (Operational Land Imager) on Landsat 9.NASA Earth Observatory/Lauren Dauphin
Its size and striking network of blue meltwater ponds offer some clues to its origin, according to Christopher Shuman, a retired University of Maryland glaciologist. Shuman thinks the berg broke from the remnant ice shelf rather than the glacier itself. Bergs calved from Zachariæ Isstrøm tend to be smaller, he said. Also, the berg’s surface—pocked with meltwater ponds, “like Swiss cheese”—closely resembles the remnant shelf ice. Past satellite images show pieces of that shelf ice drifting south and getting trapped among islands bordering the bay, where winds and tides have jostled them for years.
As of mid-August, the berg was about 1,500 kilometers (900 miles) from the bay, drifting south on the Greenland Coastal Current into the North Atlantic. Quistgaard expected the iceberg to gradually disintegrate throughout the month. Recent satellite imagery suggested it was doing just that.
Breaking up in the Denmark Strait means that remnants of the berg are unlikely to drift into busier shipping lanes that go past the southern tip of Greenland. “Its journey is a reminder of the dynamic Earth,” Shuman said, “as well as the seasonal variability of the ice in this part of the North Atlantic.”
NASA Earth Observatory images by Lauren Dauphin, using Landsat data from the U.S. Geological Survey. Story by Kathryn Hansen.
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References & Resources
NASA Earth Observatory (2015, December 4) Zachariæ Isstrøm Glacier, Greenland. Accessed August 19, 2026.
Sutherland, D. A., and Pickart, R. S. (2008). The East Greenland Coastal Current: Structure, variability, and forcing. Progress in Oceanography, 78(1), 58-77.
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The Orbital Clarity Challenge — the sixth in the NASA TechLeap Prize series — is a collaborative effort between NASA’s Heliophysics Division, Flight Opportunities program, and Center of Excellence for Collaborative Innovation. The Heliophysics Division studies space weather, including how it heats and expands Earth’s outer atmosphere during intense solar activity, creating orbital drag through atmospheric density changes. The challenge calls for low-cost methods of measuring thermospheric density, pressure, or drag in low Earth orbit. NASA is seeking approaches that are inexpensive and scalable enough to be produced in quantity and flown as hosted payloads across the commercial fleet. The challenge will unfold across three phases, advancing up to four winners’ concepts to a flight-ready solution within 12 months. At the conclusion of the challenge, NASA intends to offer each winning team a test flight at no cost.
Award: Up to four winners may receive up to $500,000 in prizes across three phases
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NASA’s Neil Gehrels Swift Observatory, shown in this artist’s concept, has orbited Earth for more than 20 years, studying the ever-changing universe.Credit: NASA’s Goddard Space Flight Center Conceptual Image Lab
Due to an ongoing commercial spacecraft attitude control issue, NASA and Katalyst Space announced Wednesday the LINK spacecraft will not capture or boost an agency satellite to a higher altitude to extend its science mission as planned. However, LINK still will attempt to conduct rendezvous and proximity operations with NASA’s Neil Gehrels Swift Observatory to demonstrate key capabilities for the future of space exploration.
“NASA should be willing to move quickly and take smart risks when the potential return is worth it, and that is exactly what we did with this mission,” said NASA Administrator Jared Isaacman. “This is not the outcome we were working toward, but it does not change why this mission was worth attempting. The team moved with extraordinary speed to give Swift a chance to carry out more science while advancing capabilities America will need for satellite servicing in the future. We are going to learn everything we can from LINK’s rendezvous attempt and put those lessons to work on the missions that follow.”
NASA and Katalyst are working closely to assess next steps for rendezvous and gather as much data as possible to inform future satellite servicing operations. “We knew this was a high-risk, high-reward mission – a first-of-its kind attempt, developed on an unprecedented timeline driven by the Sun’s activity,” said Shawn Domagal-Goldman, director, Astrophysics Division, NASA Headquarters in Washington. “We were all hoping for more science from Swift. But we knew the takeaways from this mission would be worthwhile either way, and we have gained so much through the series of accomplishments up to this point.” Without intervention, NASA anticipates Swift is likely to re-enter Earth’s atmosphere later this year. As part of the agency’s previous planning for Swift’s end of life, NASA will continue to prioritize finding new options to react rapidly to cosmic events, using current missions to help fill the gap in the meantime.
“Building, testing, and operating this mission has already strengthened America’s space industry pipeline, advancing in-space servicing capabilities in completely new ways,” Domagal-Goldman said. “NASA is committed to supporting our commercial vendors as they take on difficult tasks with the agency, to push the boundaries of what’s possible. We’re so proud of this team for: getting to the launch pad in record time, in a record-setting year for NASA astrophysics launches; its innovative problem-solving up to this point; and the dedication to the exciting capabilities this mission will attempt to demonstrate next.”
Swift was launched in 2004 to study gamma-ray bursts, the most powerful explosions in the universe, and other cosmic objects and events. It was designed for a two-year prime mission. After 21 years of science operations, Swift’s low Earth orbit began to rapidly decay because of increased solar activity. NASA used this opportunity to advance U.S. spacecraft servicing technology, awarding a contract to Katalyst in September 2025 to mount a robotic servicing mission for Swift in less than a year. The LINK spacecraft launched July 3 on a Northrop Grumman Pegasus XL rocket from Kwajalein Atoll in the South Pacific Ocean. Teams established communications with LINK and conducted in-orbit checkouts over the following weeks, before the spacecraft experienced attitude control issues.
Learn more from Katalyst, and monitor NASA’s Swift blog for continued updates throughout rendezvous:
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Alise Fisher Headquarters, Washington 202-358-2546 *****@*****.tld
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This image was taken by an Artemis II astronaut from the Orion capsule in April 2026, as the spacecraft traveled past the Moon and back over 10 days. The gray-brown, heavily cratered Moon dominates the frame against ****** space, with a partially lit crescent Earth setting behind its upper-left edge.
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Some of Earth’s microbes likely to hitch a ride to space with human explorers could survive in the shaded nooks and crannies of the Moon’s South Pole region, NASA scientists say.
Published on Aug. 19, 2026, in Science Advances, these findings highlight a need to better understand microbial persistence in extreme lunar environments. As humans build a permanent presence on the Moon, it may become difficult to distinguish ancient lunar chemistry from contamination delivered by visiting astronauts. The concern extends beyond the Moon and on to Mars, scientists say.
“Humans are natural explorers, and with them come their voices, their memories … and their microbes,” said Prabal Saxena, a planetary scientist who led the study from NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “For some scientists, myself included, that reality can be unsettling. But it also creates an opportunity to turn an imperfect situation into a useful experiment.”
Bringing microbes along is unavoidable: Humans have, on average, 1 million bacteria living on each patch of skin the size of a pencil eraser, for example. These bacteria vent from spacesuits and habitats. Though the paper’s authors worry about contamination interfering with the search for chemical clues to ancient geology or biology, they also argue that the Moon should be used as a natural lab. In shaded areas around the South Pole, scientists could carefully test the real-life limits of microbial survival in an environment that can’t easily be reproduced on Earth.
The Apollo program landed six pairs of astronauts on the Moon between 1969 and 1972. All six landing sites are near the lunar equator. In this visualization, the Apollo sites are contrasted with the South Pole, an area with enormous potential for future exploration. Time passes as we zoom toward Shackleton crater at the South Pole, revealing illumination conditions quite different from those near the equator. While many craters remain in permanent shadow, some nearby mountains and ridges are in persistent sunshine, making them attractive candidates for solar power and long-term habitation.
NASA’s Scientific Visualization Studio/Ernie Wright
Before any surface science can happen, scientists need a baseline measurement of what contaminants humans bring, the authors say.
“We need to understand what was there before us, because when we go to Mars to search for signs of life beyond our planet, we will want to make sure it’s not stuff we brought,” said Andrew Needham, a NASA Goddard-based paper co-author who is an Artemis contamination‑control scientist for lunar samples.
Even with strict sterilization procedures, some organisms are stubbornly resilient. A good example is Aspergillus ******, which is a ******* that thrives in warm, damp places like household bathrooms and heating, ventilation, and air conditioning systems. Astronauts have sampled it inside the International Space Station, and experiments demonstrate that the ******* can survive outside the station as well. Aspergillus ****** was one of five microbes, including bacteria and fungi, selected for this study because of its known toughness in spaceflight environments.
That microbes survived on the space station’s exterior surprised scientists. These species are typically not considered “extremophiles” that can withstand harsh conditions, such as the vacuum of space, according to Aaron Regberg, a geomicrobiologist at NASA’s Johnson Space Center in Houston.
“I would have expected these microbes to have dried out,” said Regberg, who studies space station bacteria and was a co-author on the paper.
NASA astronaut Kate Rubins on Oct. 14, 2016, collecting microbes in the Japanese Experiment Module aboard the International Space Station.
JAXA/Takuya Onishi
He pointed out that NASA often bakes robotic spacecraft at temperatures above 400 degrees Fahrenheit to reduce the number of living organisms on them. But that’s not possible with astronauts, so contamination concerns take on new meaning in crewed exploration of the Moon’s south polar environment.
A clearer picture of where microbes might survive comes from understanding how sunlight behaves at the poles. Survival in this study means the microbe can stay alive for at least one Earth day, which does not mean that it can grow and reproduce.
Because the Moon has a very small tilt on its axis, the view from its poles is of a Sun that appears to hover just above the horizon, skimming the surface like a flashlight laying on a table. As a result, elevated parts of the surface, including crater ridges, mountains, and even small bumps, block light from reaching low-lying terrain. This produces pockets of shadowed areas that can remain cold and preserve water, as well as shield fragile molecules and possible microorganisms from lethal radiation.
With that scientific context in mind, the team set out to test which Earth microbes could survive extreme polar conditions. They focused on organisms commonly found in spaceflight environments and those common on human skin. Besides Aspergillus ******, these included Bacillus subtilis, Staphylococcus aureus, Deinococcus radiodurans, and several species of Fusarium. Based on an analysis of previous studies, the scientists noted the maximum amount of heat and ultraviolet (UV) radiation each organism can withstand.
Then, the organisms were tested in simulations of three regions near the lunar South Pole — Nobile Rim, Connecting Ridge, and De Gerlache Rim. Those simulations used detailed environmental maps built from elevation and temperature data collected by instruments aboard NASA’s Lunar Reconnaissance Orbiter, combined with models of how radiation strikes the surface.
The models showed maps of “survivable niches” that range in size from a miles-wide crater floor to an astronaut’s boot print. Aspergillus ******, which was most resistant to UV radiation, was able to survive even in areas with some sunlight exposure. UV radiation is so deadly to most microbes that it’s used for sterilization in hospitals.
“When we think of the Moon, we don’t typically think of biology,” said Heather Graham, a paper co-author at NASA Goddard who helps develop tools and techniques for detecting biology that may look nothing like Earth’s. “But the Moon is a place where a cell can survive, so our first exploration of these sites should pay extra attention to our microbial hitchhikers and work hard to characterize lunar chemistry before our visits change what we will find.”
The authors note that while some microbes can survive in a dormant state in regions around the South Pole, and thereby confuse some future scientific investigations, there is no evidence the Moon has key ingredients to sustain growth and replication. Such ingredients include liquid water, which typically requires an atmosphere and moderate temperatures.
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International Observe the Moon Night, Sept. 19, 2026
Each year, observers around the world come together to celebrate Earth’s Moon through direct observations, hands-on activities, lunar-themed music, artwork, readings, and more.
The Moon
From lighting up our skies to preserving evidence of our solar system’s history, Earth’s closest neighbor plays a pivotal role in the study of our planet and beyond.
About the Author
Lonnie Shekhtman
Senior Science Writer
Shekhtman helps communicate NASA planetary science to the world through news and feature stories on NASA.gov, videos for NASA+ and YouTube, and by working with the media. She reports on lunar and Mars science and exploration; NASA’s search for life; missions to Venus, Titan, and Jupiter’s ******* asteroids; and many other topics related to NASA’s exploration of our solar system and beyond.
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About 12 billion years ago, a dwarf galaxy known as LKH collided with a young Milky Way and merged with it. This artist’s concept portrays that collision. NASA’s Hubble Space Telescope uncovered definitive evidence of this collision by studying globular star clusters.NASA, ESA, Joseph Olmsted (STScI)
This artist’s concept, released on Aug. 17, 2026, depicts a collision between our Milky Way galaxy and a dwarf galaxy known as LKH that happened about 12 billion years ago. A study of data from NASA’s Hubble Space Telescope, recently published in the journal Nature Astronomy, shows definitive evidence of a dwarf galaxy merging with the young Milky Way galaxy in the earliest phases of its evolution. This finding extends our knowledge of our galaxy’s history 1.8 billion years further back in time than before.
Read about this discovery.
Image credit: NASA, ESA, Joseph Olmsted (STScI)
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From left, Sean McCrary and Katie Mortensen, mechanical engineering technicians, paint NASA’s Artemis logo on the White Room connected to the crew access arm and mobile launcher inside the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on Thursday, Dec. 4, 2025. Credit: NASA/Frank Michaux
NASA has awarded approximately $10.5 million to seven institutions to help strengthen and streamline state-based pathways for students into skilled technical jobs in the aerospace industry.
The awards were made through the new NASA Aerospace Skilled Technical Workforce Hubs initiative, or NASA State Hubs. This investment in state ecosystems is designed to accelerate the development of technical roles to meet the talent demands of the space industry.
“The need for technical talent is already urgent and will only continue to grow as we return humanity to the Moon and set our sights on Mars and beyond,” said Elaine Ho, associate administrator for the Office of STEM Engagement at NASA Headquarters in Washington. “NASA is uniquely positioned to be the catalyst and convener that accelerates America’s aerospace workforce development and fosters the next generation of technicians.”
The newly awarded NASA State Hubs, represented across seven states, will function as strategic conveners that align industry employers, community colleges, high school career and technical education programs, and workforce systems to facilitate bringing students into high‑demand technical jobs, including welders, electricians, machinists, and other highly trained workers who use advanced STEM knowledge and technical skills in their occupations.
Over the next three years, the selected organizations will create programs that build critical skills identified by industry leaders, illuminate career pathways through education and apprenticeships, and build connections between employers and job seekers.
The awarded organizations are:
Antelope Valley Community College District in Lancaster, California
Georgia Tech Research Corporation
Minnesota State Colleges and Universities
Southern Utah University
Space Florida
State Board for Community Colleges and Occupation Education, Arapahoe Community College in Littleton, Colorado
Texas Space Commission
NASA State Hubs cooperative agreements are funded by the Office of STEM Engagement through its Next Gen STEM Project. The Office of STEM Engagement advances NASA’s mission by boosting the nation’s research capacity, building technical expertise, and strengthening participation in aerospace fields. The Next Gen STEM project extends this impact by preparing high school and community college students for future aerospace careers through strategic partnerships and competitive awards that develop the vital skills needed to power our Golden Age of exploration and innovation.
For more information on NASA State Hubs, visit:
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Gerelle Dodson Headquarters, Washington 202-358-1600 gerelle.q*****@*****.tld
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Related TermsLearning ResourcesNASA HeadquartersNext Gen STEMSTEM Engagement at NASA
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Career Spotlight: Mechanic (Ages 14-18)
What does a mechanic do?
Machines and engines are all around us. They power everything from cars and boats to airplanes and even rockets. Mechanics are experts who know how machinery works, especially engines, and how to fix them.
When you think of a mechanic, you might picture someone working on cars. But mechanics can be experts on all kinds of machinery.
What are some of the different types of work mechanics do at NASA?
At NASA, mechanics perform a variety of functions. For example, aerospace mechanics maintain the airplanes studied at NASA’s Armstrong Flight Research Center in Edwards, California. These might include research planes studying the environment or experimental aircraft testing new wing designs.
At NASA’s Kennedy Space Center in Florida, mechanics keep machines like the crawler-transporters in top working condition. These massive machines carry rockets from the building where they are assembled to the launch pad.
Mechanics at the agency’s Michoud Assembly Facility in New Orleans ensure the fleet of barges used to carry powerful rocket sections are maintained and ready to use. These large ships have been used for decades to carry rocket parts to various NASA centers for testing and launches.
Mechanics from Aerojet Rocketdyne inspect the engine controller of an RS-25 rocket engine at NASA’s Stennis Space Center in Mississippi.NASA
How can I become a mechanic?
There are many options that provide the training needed to get started as a mechanic. Different types of mechanics require different types of training and certifications. Here are a few examples.
Automotive mechanic: Automotive mechanics are experts at the interconnected systems in cars and trucks. After getting a high school diploma or GED, seek out trade or technical schools that have mechanic training programs. These provide hands-on experience. Further training may be required to work on specific types of automobiles. Certifications can help you advance specific skills and demonstrate proficiency.
Heavy equipment mechanic: The path to a career as a heavy equipment mechanic often begins with a two-year degree. Look for a program at your local community college or technical school. Opportunities to begin working right after high school are also available. You may start by doing basic tasks or by being paired with a senior mechanic to build skills. Most heavy equipment mechanics go through three to four years of hands-on training before taking certification and licensing tests.
Aircraft mechanic: Maintaining and repairing aircraft requires a special skillset. Community colleges and technical schools offer programs approved by the Federal Aviation Administration. These programs can fast-track your route to a career. They provide hands-on experience and help you prepare for tests needed to receive your certifications.
For many mechanic roles, military service is also a way to get training and certifications.
How can I start preparing today to become a mechanic?
In high school, take courses in math, science, and industrial technology. Check out any career and technical education programs your school might offer. Read repair manuals and look for online tutorials to figure out the basics of how machines work.
You can also gain useful experience through part-time work. Look for jobs or shadowing opportunities at your local repair shop.
Begin researching training programs, community colleges, and apprenticeship opportunities. Compare options to see which pathway seems right for you. This will help you understand program requirements and ensure you’re ready to take the next step.
Rebekah Tolatovicz, a mechanical technician lead, works inside the Artemis III Orion crew module NASA’s Kennedy Space Center in Florida.NASA
What skills will I need to be a successful mechanic?
Mechanics must be good problem solvers. Troubleshooting repairs on complex machinery requires logical thinking and patience. Being detail-oriented is critical to make sure measurements are correct and safety specifications are met.
Keeping up with the latest technology is important, too. Mechanics use computer equipment and electronic sensors to run diagnostics. And machinery technology can evolve rapidly with new advancements like electric vehicles and drones. Take initiative and stay curious.
The best part is knowing that people's safety depends on the quality of your work. It's rewarding to watch an aircraft take off with confidence, knowing you helped make it happen.
Wissam Habbal
Aircraft Mechanic, Armstrong Flight Research Center
Additional Resources
Occupational Outlook for Mechanical Engineering Technicians: Pay, Education, Job Outlook, and More (From the U.S. Bureau of Labor Statistics)
Occupational Outlook for Aircraft Mechanics: Pay, Education, Job Outlook, and More (From the U.S. Bureau of Labor Statistics)
NASA Careers
Career Spotlight: Engineer
Career Spotlight: Scientist
Career Spotlight: Technologist
Career Spotlight: Mathematician
Career Spotlight: Welder
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Behind the Lens: Meet NASA Johnson’s Photographers
NASA Johnson Space Center’s Imagery Acquisition Group poses for a group photo on Aug. 10, 2026.
Credits:
NASA/Robert Markowitz
The Imagery Acquisition Group at NASA’s Johnson Space Center poses for a group photo in Houston, Texas on Aug. 10, 2026. Back row, from left, are NASA photographers Bill Stafford, James Blair, supervisor Mark Sowa, and NASA photographers Robert Markowitz and Luna Posadas Nava. Front row, from left, are NASA photographers Morgan Gridley, Helen Arase Vargas, and former NASA photographer Josh Valcarcel.NASA/Robert Markowitz
Photographers at NASA’s Johnson Space Center in Houston have documented some of the most defining moments in human spaceflight.
From astronaut training and engineering tests to mission control operations and milestone celebrations, their images preserve the history of exploration while capturing the people and teams behind the missions shaping the next era.
Meet the photographers behind the lens and explore the stories behind the images that have helped tell NASA’s story.
Robert Markowitz
NASA photographer Robert Markowitz flies aboard a T-38 aircraft during flight operations.NASA/Robert Markowitz
Being able to help tell the human spaceflight story, frame by frame, has been an incredible adventure.
Robert Markowitz
NASA Photographer
For more than three decades, NASA photographer Robert Markowitz has documented the people and milestones that have shaped NASA’s human spaceflight program. His career has spanned the space shuttle program, 25 years of continuous human presence aboard the International Space Station, and Artemis II.
“My favorite part of this job has always come down to the range of assignments we take on and the people I get to work with every day,” Markowitz said.
One of Markowitz’s early career highlights came during the filming of “Apollo 13,” when he served as the behind-the-scenes still photographer for nearly every KC-135 zero-gravity flight. “Looking back as a 25-year-old photographer at Johnson, I don’t think I fully appreciated how unique an opportunity it was to be there documenting those moments,” he said.
Markowitz says the job has challenged him to grow as both a photographer and a communicator. Whether photographing dozens of individual portraits in a day or coordinating a 300-person group photo, each assignment has strengthened his ability to adapt, collaborate, and connect with people.
“This work has shaped not just my career, but my life,” he said. “Being part of a team that captures and preserves the story of human spaceflight continues to be one of the great honors of my time at Johnson.”
NASA’s Artemis II flight control team works on console in the White Flight Control Room in the Mission Control Center in Houston during the mission’s lunar flyby on April 6, 2026.NASA/Robert Markowitz
Former Expedition 1 crewmembers Yuri Gidzenko, Bill Shepherd, and Sergei Krikalev celebrate the International Space Station’s 25th anniversary of continuous human habitation at Space Center Houston on Jan. 19, 2026. NASA/Robert Markowitz
The Counterweight-Offload Astronaut Suited Test and Evaluation Rig is displayed in Johnson’s Space Vehicle Mockup Facility. NASA/Robert Markowitz
NASA’s Artemis II training team gathers in front of the Orion spacecraft mockup at the Space Vehicle Mockup Facility at Johnson Space Center on May 6, 2026.NASA/Robert Markowitz
Country music artist Garth Brooks performs from mission control during a live event with the Expedition 52 crew aboard the International Space Station. From left are Dina Contella, deputy manager for the International Space Station in NASA’s Low Earth Orbit Program; NASA astronaut Stephanie Wilson; Garth Brooks; and Norm Knight, Flight Operations Director. NASA/Robert Markowitz
Members of the Apollo 13 movie cast and crew take part in a zero-gravity flight aboard a KC-135 aircraft, owned by NASA at the time. Floating from left are actor Tom Hanks, who portrayed astronaut Jim Lovell; director Ron Howard; actor Bill Paxton, who portrayed astronaut Fred Haise; actor Kevin Bacon, who portrayed astronaut Jack Swigert; actor Gary Sinise, who portrayed astronaut Thomas Mattingly; and executive producer Todd Hallowell.NASA/Robert Markowitz
Bill Stafford
NASA photographer Bill Stafford photographs an event in the Teague Auditorium at NASA’s Johnson Space Center in Houston. NASA/David DeHoyos
I love figuring out how to frame a single image so it captures not just a moment, but the significance behind it.
Bill Stafford
NASA Photographer
NASA photographer Bill Stafford’s path to Johnson began during his senior year of college, when a friend who was completing a photography internship at the center told him about an opening on the photography team. With a longtime interest in science and technology, Stafford saw the opportunity to combine those interests with photography in an extraordinary environment.
Stafford approaches each assignment as a technical challenge and a storytelling opportunity. Whether working around constraints in lighting, timing, or access, he uses composition, visual psychology, and an understanding of how a viewer’s eye moves through an image to shape the final photograph.
“My favorite part of the job is the problem-solving that comes with it,” Stafford said.
Working at Johnson has sharpened those instincts as he photographs spacecraft, hardware, astronauts, and the people behind NASA’s human spaceflight missions.
“So many of the subjects I photograph carry weight and history that I want the image to reflect,” he said.
NASA astronauts Reid Wiseman (right) and Victor Glover (left) participate in an Artemis II entry simulation at NASA’s Johnson Space Center in Houston.NASA/Bill Stafford
NASA’s Joint Extravehicular Activity and Human Surface Mobility Program test team conducts a mock spacewalk to prepare for lunar surface operations and technology development for future Artemis missions.NASA/Bill Stafford
NASA astronaut and Expedition 75 Flight Engineer Anil Menon participates in photography training at NASA’s Johnson Space Center in Houston. NASA/Bill Stafford
NASA’s Exploration Extravehicular Mobility Unit is photographed inside a thermal vacuum chamber at NASA’s Johnson Space Center in Houston. NASA/Bill Stafford
Participants test technology during NASA Spacesuit User Interface Technologies for Students (SUITS) test week at NASA’s Johnson Space Center in Houston.NASA/Bill Stafford
James Blair
NASA photographer James Blair prepares to capture imagery during a flight operations assignment. NASA
I truly enjoy capturing candid photos of people during decisive moments.
James Blair
NASA Photographer
From newspapers across the country to working as a photographer and photo editor for a publication in Ecuador, NASA photographer James Blair began his career in photojournalism. Photography has taken him around the world, a path that has continued at Johnson with assignments ranging from astronaut training to geology field training in Iceland.
“Since I was very young, I have always been fascinated by spaceflight and the technology it takes to reach beyond Earth’s atmosphere,” Blair said.
At Johnson, Blair combines that fascination with his photojournalism background to document the people and technology shaping NASA’s next era of exploration.
“I enjoy documenting the new hardware that is being developed to return us to the Moon,” he said. “From spacesuits to rovers and potential lunar habitats, I get to show the world what NASA has in store for the future of human spaceflight.”
U.S. Navy divers and Artemis II astronauts aboard an inflatable raft are approached by helicopters and lifted away to the recovery ship after egressing NASA’s Orion spacecraft. NASA/James Blair
Artemis II crew members Christina Koch (middle) and Victor Glover (right) participate in an Artemis lunar imaging training using an Orion crew configuration at NASA’s Johnson Space Center.NASA/James Blair
From left, JAXA (Japan Aerospace Exploration Agency) astronaut Aki Hoshide and NASA astronaut candidates Yuri Kubo and Cameron Jones participate in an Artemis geology field training expedition in Iceland.
From left, EVA task officer Bridget Scheib, chief training officer John Ray, NASA astronaut candidate Cameron Jones, geology instructor and Artemis science officer Kelsey Young, associate research scientist Patrick Whelley, geology instructor and Artemis curation lead Juliane Gross, and JAXA (Japan Aerospace Exploration Agency) astronaut Aki Hoshide participate in an Artemis geology field training expedition in Iceland.NASA/James Blair
From left, Artemis IV chief training officer Bryce Prescott, geology instructor Jacob Richardson, and NASA astronaut Zena Cardman participate in an Artemis geology field training expedition in Iceland. NASA/James Blair
Helen Arase Vargas
NASA photographer Helen Arase Vargas captures a news conference on lunar terrain vehicles for Artemis missions at NASA’s Johnson Space Center in Houston on April 3, 2024. NASA/Robert Markowitz
I’ve always liked the idea of my work serving the public interest.
Helen Arase Vargas
NASA Photographer
NASA photographer Helen Arase Vargas began her career in photojournalism and reporting in Southern California before joining Boeing’s scientific photography team in El Segundo. Her experience photographing aerospace sparked an unexpected interest that eventually led her to Johnson.
“The best part of the job is my coworkers; cheesy, but there is so much to learn from everyone,” Arase Vargas said. “Our core team has so much knowledge. They are all quick to offer help and are great humans.”
Arase Vargas says much of the work at Johnson reflects the journalism ethics she learned early in her career and fulfills her desire to serve the public interest.
The range and volume of assignments also helped her become more comfortable working in different environments while continuing to develop her craft.
For Arase Vargas, documenting the Artemis II crew’s return to Ellington Field in Houston came with a heightened sense of responsibility.
“The world is watching, and all that imagery must be rushed out by the lab,” she said. “Your photo could be the one that ends up on every news site, and you don’t want to miss capturing the joy and celebration the moment deserves.”
NASA’s Artemis II crew returns to Ellington Field in Houston following the mission on April 11, 2026. NASA/Helen Arase Vargas
The Artemis III crew poses for an official portrait in Houston, Texas. In the back row, from left, are NASA astronauts Andre Douglas and Frank Rubio. In the front row, from left, are ESA (European Space Agency) astronaut Luca Parmitano and NASA astronaut ****** Bresnik.NASA/Helen Arase Vargas
ESA (European Space Agency) astronaut Sophie Adenot poses in an Extravehicular Mobility Unit during a portrait session at NASA’s Johnson Space Center.NASA/Helen Arase Vargas
NASA’s 2025 Astronaut Candidate Class participates in geology training at Rio Grande del Norte National Monument in New Mexico on May 20, 2026. NASA/Helen Arase Vargas
The 2025 Astronaut Candidate Class poses for a holiday photo during wilderness survival training at Fort Rucker in Alabama. NASA/Helen Arase Vargas
NASA teams conduct nighttime operations training with a Lunar Terrain Vehicle Ground Test Unit at Johnson Space Center’s Rock Yard. NASA/Helen Arase Vargas
Luna Posadas Nava
NASA photographer Luna Posadas Nava documents the Artemis II crew return at Ellington Field in Houston. NASA/Luna Posadas Nava
I have used the camera as a bridge between curiosity and understanding.
Luna Posadas Nava
NASA Photographer
NASA photographer Luna Posadas Nava’s path to Johnson spans emerging technology, optics and imaging systems, and photographing artists across the East Coast. Her work grew from a desire to visualize and expand the boundaries of what is possible.
Joining Johnson shortly before the launch of NASA’s Artemis II mission, one of Posadas Nava’s first experiences was helping bring Moon Joy to the world. She documented the Science Evaluation Room, where scientists worked together to conduct real-time lunar science observations during the mission’s lunar flyby.
Posadas Nava said it was inspiring to witness the team at work and especially meaningful to see so many women contributing to the mission’s science.
Seeing the response from women in her own life and online reinforced for Posadas Nava the power of representation through photography.
“When we see ourselves in stories, we imagine new futures,” she said. “I hope my work helps more people see themselves in the story of exploration, because what we see shapes what we believe is possible.”
The Artemis II lunar science team celebrates in the Science Evaluation Room following the mission’s successful lunar flyby. Artemis II Deputy Lunar Science Lead Marie Henderson stands at left. From the right foreground are lunar science team members Ariel Deutsch; Maria Banks, behind her; Ryan Watkins, to her right; and Sara Schmidt.NASA/Luna Posadas Nava
Artemis II deputy lunar science lead Jacob Richardson, left, and Artemis II lunar science team member Kiarre Dumes react to the astronauts’ verbal observations of the Moon during the mission’s lunar flyby on April 6, 2026.NASA/Luna Posadas Nava
Artemis II science officer Angela Garcia, left, and lunar science team member Kiarre Dumes discuss science operations in the Science Evaluation Room at NASA’s Johnson Space Center.NASA/Luna Posadas Nava
NASA engineers and teams from the Rock and Roll with NASA Challenge test rover prototypes at NASA’s Johnson Space Center Rock Yard in Houston on July 31, 2026. NASA/Luna Posadas Nava
NASA’s Artemis III crew participates in a video shoot for the crew announcement at NASA’s Johnson Space Center on June 3, 2026. NASA/Luna Posadas Nava
The Expedition 73 crew attends a debrief and awards ceremony at Space Center Houston on June 16, 2026. NASA/Luna Posadas Nava
David DeHoyos
NASA photographer David DeHoyos is photographed during an assignment in the Space Vehicle Mockup Facility at NASA’s Johnson Space Center in Houston. NASA
I am very aware of the importance of preserving history and what it means to others when our images are shared with the world.
David DeHoyos
NASA Photographer
Growing up in Houston during the Apollo era, NASA photographer David DeHoyos knew from an early age that he wanted to be part of the space industry. His interest in photography began with his mother’s Kodak Instamatic camera and continued through school and a decade working in photo labs. In 1991, that path brought him to Johnson’s photo lab and eventually behind the camera as a NASA photographer.
After more than three decades at Johnson, DeHoyos says connecting with people remains one of his favorite parts of the job. He enjoys learning about the people he photographs, sharing what he has learned about Johnson with visitors and new employees, and encouraging the next generation.
“I keep an assortment of NASA goodies in my camera bag, and the ultimate joy I get is giving a pin or sticker to a child and seeing their little faces just light up,” DeHoyos said. “It just warms my heart to encourage a youngster to work hard and pursue their dreams because that’s how I got here.”
For DeHoyos, photography is also about preserving moments that can take on greater meaning over time.
“I love the process of figuring out technical details to create an image that will make someone say, ‘Wow, cool shot, how did you do that?’” he said.
NASA’s Artemis II commander Reid Wiseman participates in emergency cabin leak training for the Orion spacecraft at NASA’s Johnson Space Center in Houston. NASA/David DeHoyos
Artemis II Pilot Victor Glover returns to Ellington Field in Houston following the crew’s nearly 10-day mission around the Moon on April 11, 2026.NASA/David DeHoyos
NASA astronaut Zena Cardman participates in emergency consultation training at NASA’s Johnson Space Center in Houston. NASA/David DeHoyos
Members of NASA Johnson’s Extravehicular Activity, Robotics, and Crew Operations Division gather for a group photo in the Neutral Buoyancy Laboratory high bay. NASA/David DeHoyos
NASA astronaut Anil Menon participates in a hardware review run at NASA’s Neutral Buoyancy Laboratory in Houston on April 23, 2025. NASA/David DeHoyos
The Honeybee Robotics prototype undergoes lunar VSAT (Vertical Solar Array Technology) testing inside Chamber A at NASA’s Johnson Space Center in Houston.NASA/David DeHoyos
About the AuthorSumer Loggins
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Astronomy Picture of the Day
Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
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Juan Pablo Castañeda
The Case of the Mysterious Maybe Meteor
Explanation: Whatdunit? What disappeared while crossing a partially eclipsed Sun? Let’s present the evidence. The 24 frames-per-second video was taken in Spain (40°34’30.3″N 1°12’28.8″W) at 20:28 local time on August 12, 2026. The Perseids meteor shower was at its peak during this time. Is this a meteor? Meteor showers trace back to a region of the sky called a radiant point that corresponds to where the Earth is crossing a comet’s path. The object’s path might trace back to the Perseids’ radiant point in the Perseus constellation. The object trails a smaller angle on the sky than the 0.5 degree Sun and Moon, which is smaller than expected for a meteor. Its brightness does not extend much past the Sun, but a meteor burning up in the sky would not need sunlight to be seen. Perhaps the sunlight is reflecting off of the object? After cross-referencing the location, time, and point in the sky with a flight database, the culprit is found to be an airplane contrail!
Tomorrow’s picture: another mystery
Date:
August 19, 2026
Credit & Copyright:
Juan Pablo Castañeda
Authors & editors:
Keighley Rockcliffe, Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti
Hat tip:
William Cooke, David Lee, Peter Brown, Denis Vida, Peter Jenniskens
A service of:
ASD at NASA / GSFC, NASA Science Activation & Michigan Tech. U.
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APOD: 2026 August 18 – Perseids from Perseus
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3 min read
NASA’s LRO Images Falcon 9 Crater on Moon, Learns New Details
This is an animated before-and-after view of the crater formed after a Falcon 9 upper stage struck the Moon’s surface on Aug. 5, 2026. These images were taken between Aug. 11 and 12 by the Narrow-Angle Camera on NASA’s Lunar Reconnaissance Orbiter. These images are enlarged three times from the original, with north facing up, and they cover an area about a quarter of a mile wide.
NASA Goddard/Intuitive Machines
Between Aug. 11 and 12, NASA’s Lunar Reconnaissance Orbiter (LRO) captured a series of images of a new crater on the Moon. The crater formed on Aug. 5, when a SpaceX Falcon 9 upper stage impacted the surface following its January 2025 launch of the Firefly Blue Ghost 1 mission.
To capture imagery of the impact, engineers tilted the spacecraft so its cameras would point toward the crater each time LRO passed about 60 miles above the Moon, traveling 1 mile per second. The orbiter circles the Moon from pole to pole every two hours, while the Moon slowly rotates underneath it. To photograph a specific spot, the spacecraft must wait until that location turns into view, which took six days in this case.
Getting the pointing right was only half the challenge; timing had to be accurate as well. If the camera snapped even 10 seconds too early or too late, the target would drift off-center by 10 miles.
An artist concept video showing NASA’s Lunar Reconnaissance Orbiter circling the Moon.
NASA’s Goddard Space Flight Center Conceptual Image Lab
Because of the variety of viewing angles, scientists could see the crater under multiple lighting conditions that revealed unique features. In images where the crater rim stood out, scientists measured its 60‑foot width. Scientists also determined the crater is less than 10 feet deep based on the length of its shadow.
To capture these details, LRO used its Narrow-Angle Camera, which can spot features as small as 3 feet wide.
Collected between Aug. 11 and 12 by NASA’s Lunar Reconnaissance Orbiter, six days after a Falcon 9 upper-stage booster impacted the Moon, these images were taken from different viewing angles, bringing out different features. The darker area that fans around the crater in the upper-left image is rougher than the surroundings, as this surface material has been altered over a long time by solar wind, galactic cosmic rays, and micrometeorite impacts. The brighter rays and splotch above the crater in the lower-right image is fresher material that was excavated from deeper below the surface. The pictures are arranged in the order they were taken, starting at the top left and moving toward the bottom right, with the lighting angle from the Sun gradually changing from one image to the next. Each image is enlarged two times and shows an area of the Moon about 1,000 feet wide.
NASA Goddard/Intuitive Machines
The images above show bright and dark rays stretching out from the crater. The darker streaks are made of surface dust and rocks altered over a long time by solar wind, galactic cosmic rays, and micrometeorite impacts. This weathered material was excavated by the collision from 1.5 feet into the lunar surface. The brighter streaks near the crater rim are made of fresh material excavated from deeper underground.
This image from NASA’s Lunar Reconnaissance Orbiter shows two oval regions where the Falcon 9 upper stage was likely to impact the Moon, based on calculations by engineers with NASA’s Center for Near Earth Object Studies. Both ellipses are 2.1 miles long and 0.4 miles wide. Both predictions use the same booster-trajectory calculations, but only the blue ellipse takes into account the lunar terrain (vs. a smooth sphere). The red and blue dots show predicted impact locations, whereas the cyan dot shows the actual impact site.
NASA/JPL-Caltech
Finding the impact site took global coordination among experts and hobbyists. Independent astronomers first identified the rocket’s trajectory using publicly available data. NASA’s Center for Near Earth Object Studies, which tracks natural objects that could pose hazards to Earth for the agency’s Planetary Defense program, used this opportunity to test and validate tools and techniques for predicting impacts.
Based at NASA’s Jet Propulsion Laboratory in Southern California, the center incrementally refined the trajectory until identifying the location of impact, which it provided to the Republic of Korea for their Korea Pathfinder Lunar Orbiter (Danuri) team. The team used the high-resolution LUTI camera on Danuri a few hours later to image the crater, finding the prediction was accurate to about 0.6 miles.
After capturing images of the crater, the Danuri mission sent coordinates to NASA’s LRO team to help refine their follow-up imaging sequence. Comparing their new crater images with the pre-impact images, the LRO team updated the crater center coordinates: 19.4759°N, 266.7138°E, 511 meters elevation.
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Last Updated
Aug 18, 2026
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Credit: National Institute of Aerospace
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“The demands for creative solutions like airborne platforms to improve the infrastructure sector are increasing exponentially,” said Steven Holz, Gateways to Blue Skies competition lead, NASA’s Langley Research Center in Hampton, Virginia. “The time is ripe for innovative students to transform how we work with our critical infrastructure, and this competition gives talented students the opportunity to do so.”
Sponsored by NASA’s University Innovation Project, the 2027 Gateways to Blue Skies competition encourages multidisciplinary teams of college students to conceptualize innovations in the world of aviation. Each year, the competition selects a new theme based on a complex challenge facing the Nation. It aims to engage as many students as possible from all backgrounds, majors, and collegiate levels.
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Image credit: NASA/James Blair
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